The Brown-York quasilocal energy transforms under conformal rescalings via Eq. (16) and under generalized Kerr-Schild maps via Eq. (34) in spherical symmetry, with no simple closed formula analogous to the Misner-Sharp-Hernandez case.
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Spacetime mappings of the Brown-York quasilocal energy
The Brown-York quasilocal energy transforms under conformal rescalings via Eq. (16) and under generalized Kerr-Schild maps via Eq. (34) in spherical symmetry, with no simple closed formula analogous to the Misner-Sharp-Hernandez case.